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Fig. 1


XMM-Newton image of observation 0679580201, with V751 Cyg marked. The bright source towards the bottom left is the chromospherically active, rapidly rotating, late-type giant star HD 199178 (V1794 Cyg; e.g., Gondoin 2004). North is up, East to the left and the rotation of the image is due to the roll angle of the spacecraft (244). The image is plotted using a log intensity scale.

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